Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
Layers in Crater in Northeast Sinus Meridiani: ESP_086244_1805 ESP_086666_1805 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.362 | 5.66 | 2.87 | -23.9 | 40.6 | 46.6 |
Fluvial Features in Noachis Terra: ESP_086350_1580 ESP_086772_1580 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.5 | 353. | 6.39 | -17.1 | 51.1 | 58.3 |
Fluvial Valley South of Ares Vallis: ESP_086311_1890 ESP_087168_1890 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.094 | 335. | 4.24 | 24.34 | 39.5 | 43.5 |
Possible Thin Glacial Lobe in Young Crater: ESP_086309_1490 ESP_086810_1490 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.4 | 35.6 | -7.9 | 3.638 | 56.9 | 63.4 |
North-Pole Facing Deposit in Crater: ESP_086354_2255 ESP_087000_2255 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.43 | 237. | -7.2 | 12.07 | 49.6 | 44.1 |
Margin of Smooth Lobate Deposit in Nereidum Montes: ESP_086259_1405 ESP_085824_1405 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.1 | 321. | -1.8 | -16.3 | 61.6 | 55.3 |
Crater and Ice-Rich Terrain: ESP_086346_2250 ESP_086992_2250 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.64 | 95.4 | -5.9 | 13.11 | 49.1 | 43.8 |
Hillslope Morphologies Southeast of Ostrov Crater: ESP_086219_1520 ESP_085375_1520 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 332. | -6.1 | 8.78 | 53.6 | 40.3 |
Head of Lethe Vallis: ESP_086199_1840 ESP_087056_1840 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.785 | 153. | 5.44 | 20.19 | 39.3 | 45.1 |
Features around Cerberus Palus: ESP_086252_1850 ESP_086819_1850 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.904 | 146. | 5.75 | -7.57 | 39.5 | 45.0 |
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